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Space Astro
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Info for exoplanet "Ketania-pina"
Scientific (actual) data |
Planet | Kepler-1622 b |
Planet status | Confirmed |
Radius | 0.131 |
Orbital period | 10.8119 |
Discovered | 2016 |
Updated | 2021-02-05 |
Tconj | 2454970 |
Publication | Announced on a website |
Detection type | Primary Transit |
Alternate names | 2MASS J19491893+4748556 b, K04765.01, KIC 10615440 b, KOI-4765 b, KOI-4765.01, WISE J194918.92+474855.6 b |
Star name | Kepler-1622 |
Right ascension | 297.33° |
Declination | 47.82° |
Mag j | 12.422 |
Mag h | 12.18 |
Mag k | 12.104 |
Star distance | 927 |
Star metallicity | 0.04 |
Star mass | 1.31 |
Star radius | 1.5 |
Star age | 2.19 |
Star temperature | 6436 |
Star alternate names | 2MASS J19491893+4748556, KIC 10615440, KOI-4765, WISE J194918.92+474855.6 |
Wikipedia article | Kepler-1622 b |
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Fictional info (?) |
Suggested name | Ketania-pina |
Planet type | Cold planet |
It is named after the deity Ketania-pina, the spirit of war.
Ketania-pina's axis has the smallest tilt of any of its solar system's planets.
It may have had oxygen oceans in the past, but these would have vaporized as the temperature rose due to a runaway greenhouse effect.
In late February 2100, Ketania-pina was visited by the New Horizons probe, which used Ketania-pina's gravity to increase its speed and bend its trajectory en route to Propa.
The Ketania-pina system has a unique configuration among those of the planets because its axis of rotation is tilted sideways, nearly into the plane of its solar orbit. |
Atmosphere | Helium | 50% |
2H2O | 33% |
Oxygen | 16% |
Atmospheric pressure | 0.03 bar |
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No known satellites |
Google search for Ketania-pina |
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Website by Joachim Michaelis
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